Published 1983 | Version v1
Book

IUE spectra of RS CVn stars

  • 1. Armagh Observatory, Northern Ireland (UK)
  • 2. Colorado Univ., Boulder (USA)
  • 3. Catania Univ. (Italy). Osservatorio Astrofisico

Description

Evidence is presented that in RS CVn stars the UV chromospheric and transition region line fluxes vary such that maximum line flux corresponds to optical minimum or maximum spot visibility. This is consistent with a solar-type dark spot model. (Auth.)

Additional details

Publishing Information

Publisher
D. Reidel.
Imprint Place
Dordrecht (Netherlands)
ISBN
90-277-1601-3
Imprint Title
Activity in red-dwarf stars
Imprint Pagination
669 p.
Journal Volume
102
Series
Astrophysics and space science library.
Journal Page Range
p. 444-445.

Conference

Title
71. Colloquium of the International Astronomical Union.
Dates
10-13 Aug 1982.
Place
Catania (Italy).

INIS

Country of Publication
Netherlands
Country of Input or Organization
Netherlands
INIS RN
15023495
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference, Numerical Data
Descriptors DEI
BINARY STARS; EMISSION SPECTRA; EXPERIMENTAL DATA; PHOTOMETRY; SPECTROSCOPY; STELLAR CORONAE; STELLAR FLARES; VISIBLE RADIATION
Descriptors DEC
ATMOSPHERES; DATA; ELECTROMAGNETIC RADIATION; INFORMATION; NUMERICAL DATA; RADIATIONS; SPECTRA; STARS; STELLAR ATMOSPHERES

Optional Information

Notes
4 figs. Imprint:Includes subject index.